J/ApJ/708/1452    Quadratic F_ij_ force field in l-CH_4_^-^      (Senent+, 2010)
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Ab initio characterization of C^-^_4_, C_4_H, and C_4_H^-^.
    Senent M.L., Hochlaf M.
   <Astrophys. J., 708, 1452-1458 (2010)>
   =2010ApJ...708.1452S
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ADC_Keywords: Atomic physics
Keywords: astrochemistry - ISM: molecules - molecular data - molecular processes

Abstract:
    Using state-of-the-art theoretical methods, we investigate the stable
    isomers of C^-^_4_, C_4_H and C_4_H^-^. Three of them are relevant for
    astrophysics and astrochemistry. These computations are performed
    using highly correlated ab initio methods and the aug-cc-pVXZ (X=T,Q)
    basis sets. In addition to the linear isomers, we predict the
    existence of several cyclic and branched forms for these molecules.
    For all the molecular species of interest here, sets of spectroscopic
    parameters are determined with perturbation theory, which compare
    quite well with experiment. For l-C_4_H^-^(X^1^{Sigma}^+^), the
    quartic force field is computed at the coupled cluster level of
    theory. This force field is derived from full nine-dimensional
    potential energy surface generated close to the equilibrium geometry
    of this anion. Finally, we treat the thermochemistry of the hydrogen
    attachment and the electron attachment reactions that may lead to the
    formation of the C_4_H^-^ from either C^-^_4_ or C_4_H.

Description:
    Electronic structure calculations have been achieved with the MOLPRO
    program suite (MOLPRO version 2002). The search of stationary points
    and determination of first-order spectroscopic parameters were
    performed at the coupled cluster including perturbative treatment of
    triple excitations ((R)CCSD(T); Knowles et al. 1993JChPh..99.5219K)
    and at the complete active space self consistent field (CASSCF;
    Knowles et al. 2000JChPh.112.3106K) levels. For these computations,
    the Dunning's basis sets including diffuse functions were employed
    (Dunning 1989JChPh..90.1007D; Kendall et al. 1992JChPh..96.6796K). The
    main group of spectroscopic parameters of the l-C_4_H^-^ anion has
    been calculated with second-order perturbation theory applied on the
    quadratic, cubic, and quartic force fields derived from a
    CCSD(T)/aug-cc-pVQZ nine-dimensional potential energy surface (PES)
    and the code FIT-ESPEC (Senent 2007ApJ...670.1510S). For CASSCF
    calculations, the active space was defined considering all the {pi}
    orbitals.

File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table4.dat     20      187  *(R)CCSD(T)/aug-cc-pVTZ quadratic F_ij_ force
                             field of l-CH_4_^-^
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Note on table4.dat: computation with the MOLPRO program suite (version 2002).
     See Knowles et al. 1993JChPh..99.5219K for (R)CCSD(T) treatment.
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Byte-by-byte Description of file: table4.dat
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   Bytes Format Units   Label     Explanations
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   1-  2  I2    ---     i         [-7/7] The i component of the force field
   4-  5  I2    ---     j         [-7/7] The j component of the force field
   7-  8  I2    ---     k         [-7/7] The k component of the force field (1)
  10- 11  I2    ---     l         [-6/7] The l component of the force field (1)
  13- 20  F8.4  ---     Term      Most significant term
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Note (1): When "k" and "l" are zero the force field is anharmonic quartic.
          When just "l" is zero the force field is cubic and when neither
          "k" and "l" are zero the force field is quartic.
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History:
    From electronic version of the journal

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(End)                 Greg Schwarz [AAS], Emmanuelle Perret [CDS]    22-Feb-2012
